Fig. 9.
Left: resulting distribution of final WD masses for LMXBs/IMXBs with 1.3 M⊙ NSs. The He WDs are the least massive, followed by hybrid WDs, and the CO WDs are the most massive. The outermost black boundary encloses the stable systems and the inner boundaries differentiate between the different WD types. Right: same as left but for LMXBs/IMXBs with 2.0 M⊙ NSs.
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